activity
20122026
most citedOn the maximum accretion luminosity of magnetized neutron stars: connecting X-ray pulsars and ultraluminous X-ray sources

226 citations · 2.4k across the 77 of their papers we have counts for

collaborators
Showing 2026Show all

11 papers · 1 filter

astro-ph.HE2026

Magnetospheric birefringence breaks the rotating-vector model and depolarises X-ray pulsars

Alexander A. Mushtukov, Sergey S. Tsygankov, Silvia Zane +4

Accreting X-ray pulsars have long been expected to show large linear polarisation below the cyclotron resonance. In the standard picture, this follows from two facts: radiative opa…

astro-ph.HE2026

Spin-disc misalignment drives periodic accretion and pulse profile asymmetry in X-ray pulsars

A. A. Mushtukov, V. Ganesh, S. S. Tsygankov +2

We investigate magnetospheric accretion in disc-fed X-ray pulsars assuming that the neutron star spin axis is not perpendicular to the disc plane. We focus on X-ray pulsars, where…

astro-ph.IM2026

EXPO: a quantum leap in fast, wide-band X-ray polarimetry for astrophysics

Paolo Soffitta, Sebastien Guillot, Ian Hutchinson +137

The Enhanced X-ray Polarimetry Observatory (EXPO) is a mission concept proposed to ESA as an M8 candidate, with a prospective launch in 2041. Building on the scientific success of…

astro-ph.HE2026

Modeling the Gravitational Wave Signal from the X-ray Pulsar Her X-1

I. D. Markozov, G. K. Pimenov, A. A. Mushtukov

The paper is devoted to modeling the gravitational waves from the X-ray pulsar Her X-1. The neutron star is considered as a freely precessing ellipsoid. The gravitational wave sign…

astro-ph.HE2026

Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required?

Sergey S. Tsygankov, Galina Lipunova, Valery F. Suleimanov +6

The final stages of outbursts in transient X-ray pulsars (XRPs), which are characterised by a significant decline in the mass accretion rate, provide valuable insight into the phys…

astro-ph.HE2026

Magnetospheric flows in X-ray pulsars II: Heating, cooling and ionization degree at sub-critical accretion

Alexander A. Mushtukov, Alexander Y. Potekhin, Valery F. Suleimanov +2

Magnetospheric accretion flows in X-ray pulsars shape their spectra, polarization, and variability. We model the thermal balance of the flow enveloping the neutron star magnetosphe…

astro-ph.HE2026★ 1 cited

Detection and luminosity-dependent evolution of the high-energy hump in the Be/X-ray pulsar 1A 1118-61

Alexander Salganik, Sergey S. Tsygankov, Sergey V. Molkov +12

Context. Accreting X-ray pulsars exhibit strong luminosity-dependent changes in their broad-band spectra. At high luminosities, their spectra are usually described by a power-law c…

astro-ph.HE2026

Rapid quasi-periodic reconfiguration of the accretion column in pulsar 1A 0535+262

Lingda Kong, Xiaohang Dai, Andrea Santangelo +12

Accretion onto strongly magnetized neutron stars is commonly interpreted using quasi-steady models, in which the accretion-column structure adjusts smoothly to the mass inflow rate…

astro-ph.HE2026

Vacuum polarization and cyclotron resonance effects on radiative transfer and plasma deceleration in subcritical X-ray pulsars

I. D. Markozov, A. Y. Potekhin, A. D. Kaminker +1

We investigate the spectrum and polarization of radiation emerging from a subcritical X-ray pulsar using self-consistent radiation-hydrodynamic simulations of an accretion channel…

astro-ph.HE2026★ 1 cited

Beaming of polarized radiation in subcritical X-ray pulsars

I. D. Markozov, A. Y. Potekhin, A. D. Kaminker +1

Radiation of X-ray pulsars is powered by accretion on the neutron star surface from a binary companion under the influence of a strong magnetic field. We study beaming of this radi…

astro-ph.HE2026

Discovery of energy-dependent phase variations in the polarization angle of Cen X-3

Qing-Chang Zhao, Lian Tao, Sergey S. Tsygankov +7

We present a detailed polarimetric analysis of Cen X-3 using \ixpe observations during its high state, revealing complex energy-dependent polarization behavior. While phase-average…